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Phonons & electron-phonon coupling

Claudia Ambrosch-Draxl Department für Materialphysik, Montanunversität Leoben, Austria Institut für Physik, Universität Graz, Austria. Phonons & electron-phonon coupling. k+q. k. q. k'-q. k'. Some important phenomena. Charge transport Heat transport Thermal expansion

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Phonons & electron-phonon coupling

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  1. Claudia Ambrosch-DraxlDepartment für Materialphysik, Montanunversität Leoben, Austria Institut für Physik, Universität Graz, Austria Phonons & electron-phonon coupling

  2. k+q k q k'-q k' Some important phenomena • Charge transport • Heat transport • Thermal expansion • Electron (hole) lifetimes • Superconductivity ? effective electron-electron interaction Aspects of e-ph Coupling

  3. Basics • The frozen phonon approach • Lattice dynamics • Atomic forces Phonons and electron-phonon coupling • Symmetry • Vibrational frequencies • Normal vectors • Raman scattering • Linear-response theory • Comparison with experiment • LAPW / WIEN2k specific aspects and examples Outline

  4. 1D case: • Harmonic approximation • Calculate energies • Fit expansion coefficients The Frozen-Phonon Approach

  5. General case: Force constant: change of the force acting on atom a in unit cell n in direction i, when displacing atom b in unit cell m in direction j. Displacement wave: The Harmonic Approximation

  6. Equation of motion: Vibrational frequencies w: by diagonalization of the dynamical matrix D • N atoms per unit cell • 3N degrees of freedom • Set of 3N coupled equations The Harmonic Approximation

  7. N atoms per unit cell • Harmonic case only! • Interpolation only – no fit! Computational Effort

  8. Many particle Schrödinger equation electronic coordinates ionic coordinates groundstate wavefunction with respect to fixed ions The Hellmann-Feynman Theorem

  9. component of the electric field caused by the nuclear charge Hellmann-Feynman force: total classical Coulomb force acting on the nucleus a stemming from all other charges of the system = electrostatic force stemming from all other nuclei + electrostatic force stemming from the electronic charges The Hellmann-Feynman Force

  10. Total energy: Atomic force: Pulay corrections Forces in DFT

  11. Hellmann-Feynman force: classical electrostatic force excerted on the nucleus by the other nuclei and the electronic charge distribution IBS force: incomplete basis set correction due to the use of a finite number of position-dependent basis functions Core correction: contribution due to the fact that for core electrons only the spherical part of the potential is taken into account Forces in the LAPW Basis

  12. Interstitial: planewave basis Atomic spheres: atomic-like basis functions site-dependent! The LAPW Method

  13. O(1) Orthorhombic cell: Pmmm Cu(1) Ba O(4) Cu(2) Y O(3) O(2) Example: YBa2Cu3O7

  14. Ag B1u B2g B2u B3g B3u Factor group analysis: q=0 5 Ag + 8 B1u + 5 B2g + 8 B2u + 5 B3g + 8 B3u Dynamical matrix Infrared-active Raman-active Bilbao Crystallographic Server: http://www.cryst.ehu.es/ Symmetry

  15. -O(2), -O(4) Force contributions for a mixed distortion: Forces in YBa2Cu3O7

  16. Ag modes YBa2Cu3O7: Phonon Frequencies

  17. Ag modes YBa2Cu3O7: Normal Vectors

  18. Ba/ Cu modes oxygenmodes YBa2Cu3O7: Lattice Vibrations

  19. Raman Active Phonons

  20. Theory Experiment CAD, H. Auer, R. Kouba, E. Ya. Sherman, P. Knoll, M. Mayer, Phys. Rev. B 65, 064501 (2002). Raman Scattering Intensities

  21. O(4) mode Probing e-ph Coupling Strength

  22. Resonance: • Peak at 2.2 eV • All oxygen modes • O(4) displacement! Probing e-ph Coupling Strength

  23. Ba-Cu modes: • Experiment: site-selective isotope substitution Probing Normal Vectors

  24. Raman scattering intensities: • Influence of mass and eigenvectors Isotope Substitution

  25. Raman scattering intensities: • Change of e-ph coupling strength through normal vectors CAD, H. Auer, R. Kouba, E. Ya. Sherman, P. Knoll, M. Mayer, Phys. Rev. B 65, 064501 (2002). • Relevant for superconductivity E. Ya. Sherman and CAD, Eur. Phys. J. B 26, 323 (2002) . Isotope Substitution

  26. Equilibrium q = 0 q ≠ 0 q-dependent Phonons

  27. Supercell method: • Unit cell commensurate with the q-vector (supercell) • Computationally very demanding Linear response theory: N. E. Zein, Sov. Phys. Sol. State 26, 1825 (1984).S. Baroni, P. Gianozzi, and A. Testa, Phys. Rev. Lett. 58, 1861 (1987). • Starting point: undisplaced structure • Treat q-dependent displacement as perturbation • Self-consistent linear-response theory • Keep single cell • Computational effort nearly independent of q-vector • Anharmonic effects neglected Supercells vs. Perturbation Theory

  28. Atomic displacement: small polarization vector • Superposition of forward and backward travelling wave • Static first-order perturbation within density-functional perturbation theory (DFPT) • Determine first-order response on the electronic charge, effective potential and Kohn-Sham orbitals Linear Response Theory

  29. Iterative solution of three equations: • Determine q-dependent atomic forces and dynamical matrix • Alternatively compute second order changes (DM) directly Linear Response Theory

  30. Electron-phonon matrix element: • Scattering process of an electron by a phonon with wavevector q Need to evaluate matrix elements like: Matrix elements including Pulay-like terms: S. Y. Savrasov and D. Y. Savrasov, Phys. Rev. B 54, 16487 (1996) . R. Kouba, A. Taga, CAD, L. Nordström, and B. Johansson, Phys. Rev. B 64, 184306 (2002). e-ph Matrix Elements

  31. Coupling constant for a phonon branch n: bcc S R. Kouba, A. Taga, CAD, L. Nordström, and B. Johansson, Phys. Rev. B 64, 184306 (2002). e-ph Coupling Constants

  32. Comparison with experiment …. • helps to analyze measured data • contributes to assign modes P. Puschnig, C. Ambrosch-Draxl, R. W. Henn, and A. Simon, Phys. Rev. B 64, 024519-1 (2001). Theory can …. • predict superconducting transition temperatures J. K. Dewhurst, S. Sharma, and CAD, 68, 020504(R) (2003);H. Rosner, A. Kitaigorodotsky, and W. E. Pickett, Phys. Rev. Lett. 88, 127001 (2002). • predict phase transitions (phonon softening) • much more …. What Can We Learn?

  33. Thank you for your attention!

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